Small-scale coronal structure, part 3

Details Small-scale coronal structure, part 3 Small-scale coronal structure, part 3

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..329w&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 329-342 (SEE N87-20871 13-92)

Physics

2

Energy Transfer, Heating, Magnetic Fields, Photosphere, Solar Corona, Solar Granulation, Sun, Extreme Ultraviolet Radiation, Microwave Emission, Models, Skylab Program, Spacelab Payloads, X Rays

Scientific paper

Recent observations and models pertaining specifically to solar coronal bright points (BPs) and generally to small-scale coronal structure are reviewed. Two questions were addressed: What is the degree of correspondence among various alleged signatures of BPs at different levels of atmosphere and what can PBs tell about the emerging flux spectrum of the sun?

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